Curvature Invariants and the Geometric Horizon Conjecture in a Binary Black Hole Merger
arXiv:2101.09615
Abstract
We study curvature invariants in a binary black hole merger. It has been conjectured that one could define a quasi-local and foliation independent black hole horizon by finding the level-- set of a suitable curvature invariant of the Riemann tensor. The conjecture is the geometric horizon conjecture and the associated horizon is the geometric horizon. We study this conjecture by tracing the level-- set of the complex scalar polynomial invariant, , through a quasi-circular binary black hole merger. We approximate these level-- sets of with level-- sets of for small . We locate the local minima of and find that the positions of these local minima correspond closely to the level-- sets of and we also compare with the level-- sets of . The analysis provides evidence that the level-- sets track a unique geometric horizon. By studying the behaviour of the zero sets of and and also by studying the MOTSs and apparent horizons of the initial black holes, we observe that the level-- set that best approximates the geometric horizon is given by .
16 pages, 4 figures; v2. included three right-hand panels to Figure 2 and updated corresponding explanations. Updated introduction and discussion for clarity. Included mention of future work in discussion/conclusion. Made various minor corrections. To appear in General Relativity and Gravitation
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